Introduction of Space Exploration Progress for Planetary Radio Burst Emission

PING Jinsong1,2, WANG Mingyuan1,2, ZHANG Mo1,2, CHEN Linjie1,2, DONG Liang2,3, WU Yuxiang1,2

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Journal of Deep Space Exploration ›› 2021, Vol. 8 ›› Issue (1) : 80-91. DOI: 10.15982/j.issn.2096-9287.2021.20200016
Article

Introduction of Space Exploration Progress for Planetary Radio Burst Emission

  • PING Jinsong1,2, WANG Mingyuan1,2, ZHANG Mo1,2, CHEN Linjie1,2, DONG Liang2,3, WU Yuxiang1,2
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Abstract

At low frequency electron-magnetic wave band, planetary bodies not only emit thermal radiation, but also emit non-thermal radiation burst. The typical emission is planetary auroral radio burst consists of planetary kilometric wave burst, Jovian radiation at hectometer and decameter wavelengths. This kind of burst has been observed on the ground and in the space for dozens of years. The developed method can also be used as remote sensing tool to detect the inner structure of Jovian magnetosphere. However, the characteristics and mechanism have not been fully understood for the solar system planetary radio burst, there are still quite a lot of open questions left. Similar radio burst may also be observed from the exoplanetary systems. Following the development of space technology, radio astronomical observation has extended to kilometer wave. In the future the large radio array at low frequency can play key role to uncover the mechanism for the planetary radio burst, and also can be used to detect the exoplanets. The Chang’e-4 lunar mission with its low frequency payloads is working as pathfinder for the Earth Auroral Kilometer Radiation (AKR) and Jovian bursts,

Keywords

planet / radio burst / aurora / Earth / Jupiter

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PING Jinsong, WANG Mingyuan, ZHANG Mo, CHEN Linjie, DONG Liang, WU Yuxiang. Introduction of Space Exploration Progress for Planetary Radio Burst Emission. Journal of Deep Space Exploration, 2021, 8(1): 80‒91 https://doi.org/10.15982/j.issn.2096-9287.2021.20200016

References

[1] BARROW C H,MORROW D P. The polarization of the Jupiter radiation at 18 Mc/s[J]. The Astrophysical Journal,1968,152:593-608
[2] BAHNSEN A,PEDERSEN B M,JESPERSEN M,et al. Viking observations at the source region of auroral kilometric radiation[J]. Journal of Geophysical Research,1989,94:6643-6654
[3] GALOPEAU P,ORTEGA-MOLINA A,ZARKA P. Evidence of Saturn's magnetic field anomaly from SKR high-frequency limit[J]. Journal of Geophysical Research,1991,96:14129-14140
[4] ZARKA P. Auroral radio emissions at the outer planets:observations and theories[J]. Journal of Geophysical Research,1998,103(E9):20159-20194
[5] DESCH M D. Does solar radio emission trigger SKR?[M]//Planetary Radio Emissions. Vienna:Austrian Acad. Sci. Press,1998.
[6] BENEDIKTOV E A,GETMANTSEV G G,SAZONOV Y A,et al. Preliminary results of measurements of the intensity of distributed extraterrestrial radio frequency emission at 725 and 1525 kHz[J]. Issled,1965,1:614
[7] VAN HAARLEM M P. LOFAR:the low frequency array[J]. EAS Publications Serries,2005,15(7):431-444
[8] 梅丽,苏彦,周建锋. 极低频射电天文观测现状与未来发展[J]. 天文学报,2018,15(2):127-139
MEI L,SU Y,ZHOU J F. The history and development of the low frequency radio observation[J]. Astronomical Research & Technology-Publications of National Astronomical Observatories of China,2018,15(2):127-139
[9] BENTUM M J,VERMA M K,RAJAN R T,et al. A roadmap towards a space-based radio telescope for ultra-low frequency radio astronomy[J]. Advances in Space Research,2020,65(2):856-867
[10] ENSON R F,AKASOFU S I. Auroral kilometric radiation/aurora correlation[J]. Radio Science,1984,19:527
[11] GURNETT D A. The Earth as a radio source:terrestrial kilometric radiation[J]. Journal of Geophysical Research,1974,79:4227
[12] WU C S,LEE L C. A theory of terrestrial kilometric radiation[J]. The Astrophysical Journal,1977,230:621-626
[13] GURNETT D A,GREEN J L. On the polarization and origin of auroral kilometric radiation[J]. Journal of Geophysical Research,1978,83:689
[14] GURNETT D A. High latitude electromagnetic plasma wave emissions[M]//High Latitude Space Plasma Physics. New York:Springer,1983:355-375.
[15] MATSUMOTO H,NAGANO I,ANDERSON R R,et al. Plasma wave observations with GEOTAIL spacecraft[J]. Journal of Geomagnetism and Geoelectricity,1994,46:59-95
[16] MORIOKA A,MIYOSHI Y,KURITA S,et al. Universal time control of AKR:Earth is a spin-modulated variable radio source[J]. Journal of Geophysical Research,2013,118:1123-1131
[17] GREEN J L,BOARDSEN S,GARCIA L,et al. Seasonal and solar cycle dynamics of the auroral kilometric radiation source region[J]. Journal of Geophysical Research,2004,109:A05223
[18] KAISER M L. Observations of non-thermal radiation from planets[C]//Plasma Waves and Instabilities at Comets and in Magnetospheres. Washington,DC:AGU,1989.
[19] MUTEL R L,GURNETT D A,CHRISTOPHER I W,et al. Locations of auroral kilometric radiation bursts inferred from multispacecraft wideband Cluster VLBI observations.1:description of technique and initial results[J]. Journal of Geophysical Research,2003,108(A11):1398
[20] KAISER M L,DESCH M D. Radio emissions from the planets Earth,Jupiter and Saturn[J]. Reviews of Geophysics,1984,22:373-384
[21] KAISER M L,DESCH M D,CONNERNEY J E P. Radio emission from the magnetic equator of Uranus[J]. Journal of Geophysical Research,1989,94:2399-2404
[22] READ P L,DOWLING T E,SCHUBERT G. Saturn’s rotation period from its atmospheric planetary-wave configuration[J]. Nature,2009,460:608-670
[23] GURNETT D A,LECACHEUX A,KURTH W S,et al. Discovery of a north-south asymmetry in Saturn’s radio rotation period[J]. Geophysical Research Letters,2009,36:L16102
[24] GURNETT D A,GROENE J B,PERSOON A M,et al. The reversal of the rotational modulation rates of the north and south components of Saturn kilometric radiation near equinox[J]. Geophysical Research Letters,2010,37:L24101
[25] DOUGHERTY M K,CAO H,KHURANA K K,et al. Saturn's magnetic field revealed by the Cassini Grand Finale[J]. Science,2018,362(6410):46
[26] LELLOUCH E,MCGRATH M E,JESSUP K L. Io's atmosphere[M]//Io After Galileo :a New View of Jupiter’s Volcanic Moon. [S. l.]:Springer Praxis Publishing Ltd,2007:231-264.
[27] ZARKA P,FARGES T,RYABOV B P,et al. A scenario for Jovian S-bursts[J]. Geophysical Research Letters,1996,23(2):125-128
[28] LADREITER H P,ZARKA P,LECACHEUX A. Direction-finding study of Jovian hectometric and broadband kilometric radio emissions:Evidence for their auroral origin[J]. Planetary and Space,1994,42:919-931
[29] KIMURA T,TSUCHIYA F,MISAWA H,et al. Radiation characteristics of quasi-periodic radio bursts in the Jovian high-latitude region[J]. Planetary and Space Science,2008,56(15):1967-1976
[30] MORIOKA A,NOZAWA H,MISAWA H,et al. ,Rotationally driven quasi-periodic radio emissions in the Jovian magnetosphere[J]. Journal of Geophysical Research,2006,111:A04223
[31] BHATTACHARYA A B,RAHA B. Detection of radio emissions from Jupiter[J]. OJP,2013,5(1-2):1-12
[32] GURNETT D A,KURTH W S,HOSPODARSKY G B,et ak. Control of Jupiter's radio emission and aurorae by the solar wind[J]. Nature,2002,415:985-987
[33] HOSPODARSKY G B,KURTH W S,CECCONI B,et al. Simultaneous observations of Jovian quasi-periodic radio emissions by the Galileo and Cassini spacecraft[J]. Journal of Geophysical Research,2004,109:A09S07
[34] BROWN S,JANSSEN M,ADUMITROAIE V,et al. ,Prevalent lightning sferics at 600 megahertz near Jupiter's poles[J]. Nature,2018,558:87-90
[35] HIGGINS C A,CARR T D,REYES F. A new determination of Jupiter's radio rotation period[M]//Planetary Radio Emissions IV.Vienna:Austrian Acad. Sci. Press,1997:43-50.
[36] WINTERHALTER D,KUIPER T,MAJID W,et al. Search for radio emissions from extrasolar planets:the observation campaign[M]//Planetary Radio Emissions VI. Vienna:Austrian Academy of Sciences Press,2006.
[37] ZARKA P. The search for exoplanetary radio emissions,in Planetary Radio Emissions VⅡ[M].Vienna:Austrian Academy of Sciences Press,2011:287-301.
[38] SIROTHIA S K,DES ETANGS A L,KRISHNA G,et al. Search for 150 MHz radio emission from extrasolar planets in the TIFR GMRT Sky Survey[J]. A&A,2014,562(2):A108
[39] SHIMWELL T W,HAVERKORN M,CSEH D,et al. The LOFAR two-metre sky survey:I. survey description and preliminary data release[J]. Astronomy & Astrophysics,2017,598:A104
[40] DES ETANGS A L,SIROTHIA S K,KRISHNA G,et al. Hint of 150 MHz radio emission from the Neptune-mass extrasolar transiting planet HAT-P-11b[J]. Astronomy & Astrophysics,2013,552:A65
[41] VEDANTHAM H K,CALLINGHAM J R,SHIMWELL T W,et al. Coherent radio emission from a quiescent red dwarf indicative of star–planet interaction[J]. Nature Astronomy,2020,4:577-583
[42] 薛长斌,周晴,王雷,等. “嫦娥4号”任务有效载荷系统设计与实现[J]. 深空探测学报(中英文),2017,4(6):515-521
XUE C B,ZHOU Q,WANG L,et al. Design and implementation of payload system in Chang’e–4 mission[J]. Journal of Deep Space Exploration,2017,4(6):515-521
[43] 贾瑛卓,邹永廖,薛长斌,等. 嫦娥四号任务科学目标和有效载荷配置[J]. 空间科学学报,2018,38(1):118-130
JIA Y Z,ZOU Y L,XUE C B,et al. Scientific objectives and payloads of Chang’ E-4 mission[J]. Chinese Journal of Space Science,2018,38(1):118-130
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